The surface temperature of the Sun is 5800 K. The mean radiuses of the Earth and the Sun are 6.37x106 m and 6.96x108 m, respectively. The average Earth-Sun distance 1.496x10¹1 m. 20 (a) Assume that both the Sun and the Earth are perfect blackbody, calculate the steady-state surface temperature of the Earth. (b) What are the peak wavelengths of radiations from the Sun and the Earth? (a) Some gases in atmosphere block a small portion of sun radiation, but are quite opaque to infrared light. Recalculate the steady-state temperature of the Earth, assume that the transmission efficiency of the atmosphere is 80% and 50% for visible and infrared light, respectively.

Principles of Physics: A Calculus-Based Text
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Author:Raymond A. Serway, John W. Jewett
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Chapter28: Quantum Physics
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helo, i need solution for this problem please, especially the last part c. thanks

The surface temperature of the Sun is 5800 K. The mean radiuses of the
Earth and the Sun are 6.37x106m and 6.96x108 m, respectively. The average Earth-Sun distance
1.496x10¹1 m.
(a) Assume that both the Sun and the Earth are perfect blackbody, calculate the steady-state
surface temperature of the Earth.
(b) What are the peak wavelengths of radiations from the Sun and the Earth?
(a) Some gases in atmosphere block a small portion of sun radiation, but are quite opaque to
infrared light. Recalculate the steady-state temperature of the Earth, assume that the
transmission efficiency of the atmosphere is 80% and 50% for visible and infrared light,
respectively.
Transcribed Image Text:The surface temperature of the Sun is 5800 K. The mean radiuses of the Earth and the Sun are 6.37x106m and 6.96x108 m, respectively. The average Earth-Sun distance 1.496x10¹1 m. (a) Assume that both the Sun and the Earth are perfect blackbody, calculate the steady-state surface temperature of the Earth. (b) What are the peak wavelengths of radiations from the Sun and the Earth? (a) Some gases in atmosphere block a small portion of sun radiation, but are quite opaque to infrared light. Recalculate the steady-state temperature of the Earth, assume that the transmission efficiency of the atmosphere is 80% and 50% for visible and infrared light, respectively.
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